1.2E-10 Watts/n 1E-10 8E-11 Energyloss 6E-11 4E-11 2E-11 P0 (mTorr) Fig. 8. Energylossrate per unitdensity vs. pressure. ... where µi is the Ar+ mobility in neutral argon and is proportional to the pressure p0. As a rough approximation, we may take |∇n / n| ≈ 1/2a, a being the discharge radius. The outward flux is then the minimum of Eqs. (3) and (8), as shown

preliminary numerical trials, leading to the production of acoustic energy ... are initiated with a half-wavelength pressure distribution of 0.5kPa in amplitude, with base pressure and temperature of 101325 Pa and 300 K. Spurious high frequency perturbations

2 dr i /dt. This assumes a constant i rate of loss of latent heat and gives ... caused by pressure changes; the rest comes from cooling. Units are: dT/dt in K Gyr ... u a of energy: it is merely a faster rate of release of latent heat. Cooling produces a contraction of 5–10 km in 1 Gyr for these models. The density and pressure both increase

2 dr i /dt. This assumes a constant i rate of loss of latent heat and gives ... caused by pressure changes; the rest comes from cooling. Units are: dT/dt in K Gyr ... u a of energy: it is merely a faster rate of release of latent heat. Cooling produces a contraction of 5–10 km in 1 Gyr for these models. The density and pressure both increase

has shrunken somewhat, as expected from the loss of pressure support in the radial ... adiabats than that of the star, primarily because less gravitational energy is available to the rotationally supported material of the disk, and energy is more readily ... and cool models. The upper portion of the Ðgure shows the meridional density contours

of the density when the pressure is within the range [Pmin , Pcrit ]. Iso-cooling contours ...loss by radiation is small compared to the increase in internal energy ... that at the centre, after a transient over-pressure, the density increases sharply while

in this study (10.9 –22.7 C). MO2 was then converted to energyloss (J) via the energy ... and was thereby subtracted from the initial energydensity in the ocean to determine ﬁnal energydensities on entrance to subnatal watersheds. We found that the rank order